FIELD OF THE INVENTION
[0001] The invention relates to a method for correcting a drift of an isotopic ratio derived
from data measured by a multi-collector mass spectrometer.
BACKGROUND ART
[0002] Evaluation of isotopic ratios of a given element is an important source of information
on the origin and transformation of a material. Isotopic analysis plays a leading
part in the nuclear industry. It is also used in numerous fields, such as biochemistry,
pharmacology, environment monitoring, criminal or food fraud fighting, geochemistry
or cosmochemistry.
[0003] Measurement of isotopic ratios in a chemical element is generally made by mass spectrometry.
Suitable instruments for these measurements are MC-ICPMS spectrometers (Multi Collector
Inductively Coupled Plasma Mass Spectrometry) because of their low limit of detection,
their high ionization potential, and simultaneous isotope analysis. These instruments
offer isotopic ratio measurements on a large range of elements.
[0004] In order to eliminate possible isobaric interferences due to different elements having
similar atomic masses in a sample, the sample to be measured should be treated by
a separation technique before being introduced into the MC-ICPMS spectrometer. To
that end, the MC-ICPMS spectrometer can be coupled with a variety of introduction
systems which usually are: High Performance Liquid Chromatography (HPLC), Ion Chromatography
(IC), Gas Chromatography (GC), Gold Trap (GT), Capillary Electrophoresis (CE) or lsoTachoPhoresis
(ITP).
[0005] For
in situ micro-analysis of solids or single micrometric particle size analysis, the MC-ICPMS
can also be coupled with the Laser Ablation technique (LA).
[0006] Online coupling between these sample introduction systems and the MC-ICPMS spectrometer
provides transient signals with specific time windows generally varying between some
milliseconds to minutes in which the isotope ratios should be accurately measured.
[0007] However, most experiments reveal a systematic increase or decrease of the point by
point isotope ratio during the transient signal, also called "isotopic ratio drift".
Most commonly used methods for the isotope ratio calculation on transient signal (point
by point method, linear regression method and Peak Area Integration method) do not
correct this isotope ratio drift which significantly degrades the quality (i.e. repeatability
and trueness) of the obtained measurements. According to the point by point method,
the isotope ratio is determined for several points of a selected peak area centered
around the maximum of the peak. The area of calculation is selected based on the stability
of the measured isotope ratio. According to the linear regression method, the isotope
ratio is given by the slope of the linear regression line which is the best fitting
line through the data points obtained by plotting the signal intensities of the two
isotopes as a function of one another. According to the Peak Area Integration method,
the isotope ratio is obtained by dividing the integrated peak areas for the two isotopes.
[0008] For explaining the origin of this drift, one hypothesis is that the isotopic ratios
derived from rapidly rising or decreasing signals are affected by responses of the
mass spectrometer Faraday amplifiers. Depending on which amplifiers are faster or
slower, measured signals become enhanced or reduced relative to each other.
[0009] In order to try to solve this problem, spectrometer constructors generally provide
a calibration technique allowing the user to adjust
tau-correction required for each of the Faraday amplifiers. Signal decay curves must first
be empirically determined for each Faraday amplifier and then applied to remove residual
bias resulting from prior signal variations from the individual readings.
[0010] However, such a calibration technique is generally not sufficient to completely remove
the isotopic ratio drift. Even after
tau-correction, time response of the different Faraday-amplifier systems may not be perfectly
uniform and remaining isotope ratio drift in transient signals may be observed.
[0011] These remaining isotope ratio time variations could be attributed to residual capacities
of the Faraday-amplifier systems due to the instrumental setup, the length and the
geometry of the wiring between the collectors. These residual capacities called stray
capacities can cause a lowering of the amplification system response and can vary
among the individual Faraday-amplifiers.
[0012] There is thus a need for a method allowing the synchronization of the Faraday-amplifier
signal responses providing an efficient correction of the isotopic ratio drift, also
capable to enhancing repeatability or reducing uncertainty of isotopic ratio analysis.
Such advantages can be of utmost importance when samples are in such quantities that
only few analyses are allowed.
SUMMARY OF THE INVENTION
[0013] One aim of the invention is to provide an efficient method for correcting the drift
of an isotopic ratio measured by a multi-collector mass spectrometer.
[0014] To that aim, the invention provides a method for correcting a drift of an isotopic
ratio in a sample, on the basis of a first signal and a second signal derived from
data measured by a multi-collector mass spectrometer, the first signal representing
a variation of a detected quantity of a first isotope in the sample as a function
of time, and the second signal representing a variation of a detected quantity of
a second isotope in the sample as a function of time, said method comprising steps
of:
- applying to the second signal a time offset so as to obtain a second offset signal,
- computing values of isotopic ratio between the first signal and the second offset
signal at a plurality of times,
- computing an isotopic ratio variation parameter as a function of the computed values
of isotopic ratio,
- adjusting the time offset applied to the second signal and repeating the preceding
steps so as to determine a time offset for which the isotopic ratio variation parameter
is reduced.
[0015] Introduction of a time offset allows adjusting the electronic hysteresis between
the different amplifiers of the mass spectrometer. Such an adjustment is made after
acquisition of the data and thus, does not require preliminary calibration of the
mass spectrometer (i.e. technique for compensating the signal decay in the Faraday-amplifiers
called
"tau-correction").
[0016] The proposed method allows quantifying and correcting precisely the time offset between
the different signals generated by the different amplifiers of the mass spectrometer,
and thus provides an efficient correction of the isotopic ratios.
[0017] Moreover, the method uses the isotopic ratios between two signals, and not the intensity
signal of each isotope independently. This allows a very precise calculation of the
time offset and therefore, a fine correction of the isotopic ratio drift.
[0018] The method can be applied to each additional data, taking into account their specificity
(such as the slope of the increase and decrease of the signal and the duration of
the transient signal), as well as the variability of the hysteresis which may possibly
vary between the different spectra (for instance depending on the intensity of the
measured signals).
[0019] The proposed method can comprise a step of:
- computing the second signal by interpolation of second data representing detected
quantities of a second isotope, measured in the sample at different times.
[0020] In particular, the interpolation can be a piecewise polynomial interpolation, preferably
a third degree piecewise polynomial interpolation.
[0021] The steps of the method can be applied to a number N of signals, N>2, each i-th signal
representing a variation of a detected quantity of a i-th isotope in the sample as
a function of time, so as to determine a time offset for each of the second to the
N-th signals.
[0022] According to a first embodiment of the invention, the isotopic ratio variation parameter
is a slope as a function of time of a straight line obtained by linear regression
of the values of isotopic ratio.
[0023] According to a second embodiment of the invention, the isotopic ratio variation parameter
is a relative standard deviation of the isotopic ratio values.
[0024] The method can comprise a step of:
- selecting a time interval in which the values of isotopic ratio are computed.
[0025] The steps can be carried out on several time intervals, and a time offset is determined
for each time interval.
[0026] The proposed method can comprise preliminary steps of:
- introducing a sample into the multi-collector mass spectrometer, and
- measuring data from the sample, the data being measured by the spectrometer.
[0027] In particular, the multi-collector mass spectrometer is coupled to an ion source.
Such an ion source may be selected from the group consisting in a thermal ionization
device, an electron ionization device and a plasma ionization device. In a preferred
embodiment, the ion source is an inductively coupled plasma device. Hence, in a more
preferred embodiment, methods of the invention can be applied to data measured by
a multi-collector inductively coupled plasma mass spectrometer (MC-ICPMS), a multi-collector
thermal ionization mass spectrometer (MC-TIMS) or an Isotopic Ratio mass spectrometer
(IRMS).
[0028] In particular, the multi-collector mass spectrometer may be coupled to a separation
system for separating the sample into several elementary fractions and successively
introducing the elementary fractions into the spectrometer.
[0029] Such a separation system may be a liquid chromatography, high performance liquid
chromatography, ion chromatography, gas chromatography, gold trap, capillary electrophoresis
or isotachophoresis.
[0030] Alternately, for
in situ isotope analysis the multi-collector mass spectrometer can also be coupled to a Laser
Ablation (LA) system and for low sample volumes analysis to a flow injection (FI)
system.
PRESENTATION OF THE DRAWINGS
[0031] The invention will be described with reference to the drawings, in which:
- Figure 1 diagrammatically shows a multi-collector mass spectrometer comprising a data
collection and processing unit programmed for carrying out a method for correcting
a drift of an isotopic ratio, according to a possible embodiment of the invention,
- Figure 2 diagrammatically shows different steps of the method for correcting a drift
of an isotopic ratio,
- Figures 3A and 3B diagrammatically shows transient signals Ia(ti) and Ib(ti) of a given element X, and a linear positive drift of the isotopic ratio when
no correction is applied (Figure 3A), and the isotopic ratio when a correction is
applied (Figure 3B),
- Figures 4A to 4C respectively show the linear increasing of values of the isotopic
ratio 208Pb/206Pb measured point-by-point (Figure 4A), values of the isotopic ratio 208Pb/206Pb after correction with a method according to the invention (Figure 4B), and a comparison
of the first embodiment of the method based on the slope obtained by linear regression
of the values of isotopic ratio and the second embodiment of the method based on a
relative standard deviation of the values of isotopic ratio (Figure 4C), wherein data
were acquired using flow injection and demountable direct injection high efficiency
nebulizer (d-DIHEN) in the Neptune MC-ICPMS,
- Figures 5A to 5D respectively show Pb transient signals acquired using flow injection
and d-DIHEN in the Neptune MC-ICPMS with an integration time (it) of 0.262 seconds
(Figure 5A), corresponding time corrected isotope ratios (Figure 5B), Pb transient
signals acquired with an integration time of 1.049 seconds (Figure 5C) and corresponding
time corrected isotope ratio (Figure 5D),
- Figures 6A to 6D respectively show a Pb transient signal acquired using a GC directly
coupled with a Nu MC-ICPMS and isotope ratios before and after drift correction of:
208Pb/206Pb (Figure 6A), 207Pb/206Pb (Figure 6B) and 204Pb/206Pb (Figure 6C), as well as slope values before (Sb) and after (Sa) isotope ratio drift correction, and Δtmin values for the Slope and RSD models for the 208Pb/206Pb, 207Pb/206Pb and 204Pb/206Pb isotope ratios (Figure 6D),
- Figures 7A to 7D respectively show three isotope plots for the GC-MC-ICPMS: 208Pb/206Pb versus 207Pb/206Pb (Figure 7A) and 208Pb/206Pb versus 204Pb/206Pb (Figure 7B), and point by point percentage relative deviations from the Exponential
Mass Fractionation Law for a given 208Pb/206Pb ratio of: 207Pb/206Pb (Figure 7C) and 204Pb/206Pb (Figure 7D),
- Figures 8A and 8B show blank-corrected and mass fractionation-corrected 207Pb/206Pb (Figure 8A) and 204Pb/206Pb (Figure 8B) isotope ratios of GC-MC-ICPMS thirty injections, all data having been
treated before and after isotope ratio drift correction with Point by Point (PbP),
Linear Regression (LR) and Peak Area Integration (PAI) methods.
DETAILLED DESCRIPTION OF AN EMBODIMENT OF THE INVENTION
[0032] Referring to figure 1, the multi-collector mass spectrometer comprises a control
unit 1, a separation and/or an injection system 2, an ion source 3, a magnetic sector
4, a multi-collector array 5 and a data collection and processing unit 6.
[0033] The control unit 1 is capable of controlling hardware and software components of
the mass spectrometer. Such a control unit 1 may be a computer. The separation and/or
an injection system 2 is a device which introduces a small amount of sample into the
ion source 3 through an inlet. The ion source 3 is used for converting a portion of
the sample into charged particles such as atomic ions. Such an ion source may be a
plasma source, a gas source or a thermal ionization source. The magnetic sector 4
allows the separation of the ions by charge to mass ratios. The multi-collector array
5 is a ion collector, typically having an array of detector-amplifiers (or Faraday
cups), which allows simultaneous detection of multiple isotopes. The data collection
and processing unit 6 is configured to process and store data measured by the multi-collector
array. It can comprise a computer for processing the data and a storage unit for storing
the measured and processed data. Moreover, the data collection and processing unit
6 is programmed for correcting a drift of an isotopic ratio in the sample according
to a possible embodiment of the method for correcting the drift of an isotopic ratio.
[0034] Chemical components which may be subjected to isotopic ratio measurements comprise
rare earth elements, alkaline earth metals, transition metals and actinides.
[0035] Referring to figure 2, different steps of a method 100 for correcting a drift of
an isotopic ratio are illustrated.
[0036] According to a first step 101, a sample is introduced into a multi-collector mass
spectrometer (MC-MS).
[0037] To that end, the multi-collector mass spectrometer may be coupled to a separation
system, such as a liquid or a gas chromatography system, a Gold Trap (GT), a Capillary
Electrophoresis (CE) or a IsoTachoPhoresis (ITP) for separating the sample into several
elementary fractions and successively introducing the elementary fractions into the
spectrometer.
[0038] In case the material to be tested is a solid, the multi-collector mass spectrometer
may be coupled to a laser ablation system for
in situ analysis, or to a flow injection system for low volume sample analysis.
[0039] The multi-collector mass spectrometer comprises several detector-amplifier systems,
each detector-amplifier being configured to measure a quantity of a given isotope
in the sample.
[0040] According to a second step 102, data from the sample are acquired by the detector-amplifier
systems of the mass spectrometer. The acquired data may comprise data measured for
a number N of isotopes in the sample (N≥2).
[0041] In the example illustrated, on figure 2, data are measured for two isotopes a and
b.
[0042] The acquired data comprises first data and second data.
[0043] The first data comprise quantities of a first isotope (isotope a) measured by a first
detector-amplifier system at different times.
[0044] The second data comprise quantities of a second isotope (isotope b) measured by a
second detector-amplifier system at different times.
[0045] Figure 3A shows an example of first data (I
a) for the isotope a, second data (I
b) for the isotope b, and values of isotopic ratio I
b/I
a of an element X at the different times t
i.
[0046] The acquired data are processed by the data collection and processing unit which
may be part of the mass spectrometer or may be separated from the mass spectrometer.
The data collection and processing unit is programmed for applying subsequent steps
of the method.
[0047] A first signal I
a is defined as being the first data representing detected quantities of the first
isotope a, measured in the sample at different times t
i. The first signal is thus composed of discrete measurement results with their associated
timestamp reads.
[0048] According to a third step 103, the data collection and processing unit computes a
second signal I
b by interpolation of second data representing detected quantities of a second isotope
(b), measured in the sample at different times.
[0049] Preferably, the second signal I
b(t) is computed by piecewise polynomial interpolation of the second data representing
detected quantities of the second isotope b, measured in the sample at different times
t
i.
[0050] According to such piecewise polynomial interpolation, a series of third polynomial
curves through the successive points of the data (i.e. piecewise) is interpolated,
which permits to create a well-behaved curve (no oscillations that are not supported
by the data) rather than to generate a single polynomial.
[0051] The third interpolation order is preferred because it is the lowest order polynomial
for which curvature can be continuous. Lower order polynomials can be used but the
result may be a jagged curve if there are many changes in slope.
[0052] Figure 3B shows an example of a second signal I
b(t
i) together with its interpolated curve I
b(t) and corresponding values of drift corrected isotope ratio I
b/I
a of an element X at different times t
i.
[0053] According to a fourth step 104, a time interval is selected in which a correction
is to be applied.
[0054] To that end, the data collection and processing unit may display a diagram showing
first and second signals I
a(t) and I
b(t), so that the user may select a time interval.
[0055] Alternatively, the data collection and processing unit may select automatically an
appropriate time interval.
[0056] Additionally, the selection can be performed several times at several stages of the
method.
[0057] As illustrated on figure 3A, an example of selected time interval is [t
1, t
3].
[0058] Within this time interval, the variation of the isotope ratio I
b/I
a as a function of time may be modeled by a linear function having a slope S defined
by:

where n is the number of isotope ratio values for computing the slope S, and t
i are the timestamp read.
[0059] Optionally, a reunion of several time intervals can be selected.
[0060] According to a fifth step 105, the data-collection and processing unit applies a
time offset Δt to one of the signals computed by interpolation, typically the second
signal according to the embodiment described and illustrated, so as to obtain a second
offset signal (I
b(t+Δt)).
[0061] In the case of several time intervals, a time offset can be determined for each time
interval, the time offset being possibly different from one time interval to another.
[0062] According to a sixth step 106, the data collection and processing unit computes values
of isotopic ratio, from the first signal I
a(t) and the second offset signal I
b(t+Δt) at a plurality of times t
i within the time interval.
[0063] For a given time t
i, the isotopic ratio is computed as a ratio of the intensity of the second signal
I
b(t
i+Δt) on the intensity of the first signal I
a(t
i). Alternatively, the isotopic ratio could be calculated as a ratio of the intensity
of the first signal I
a(t
i+Δt) on the intensity of the second signal I
b(t
i). Alternatively, the isotopic ratio could be calculated as a ratio of the intensity
of the first signal I
a(t
i) on the intensity of the second signal I
b(t
i+Δt).
[0064] According to a seventh step 107, the data collection and processing unit computes
an isotopic ratio variation parameter as a function of the values of isotopic ratios
computed during the fifth step 106.
[0065] Steps 105 and 106 can typically be performed during step 107.
[0066] The isotopic ratio variation parameter is preferably chosen so as to be easily computed.
The isotopic ratio is typically chosen so as to avoid highly divergent isotope ratio
values, for instance by an adapted normalization.
[0067] According to a first embodiment, the isotopic ratio variation parameter includes
the absolute value of the slope S of a straight line obtained by linear regression
of isotopic ratio values.
[0068] An example of such an isotopic ratio variation parameter is typically defined as
follows by formula [2]:

where Δt is the time offset applied to the second signal and n is the number of isotope
ratio values for computing the slope S.
[0069] According to a second embodiment of the invention, the isotopic ratio variation parameter
includes a relative standard deviation of the values of isotopic ratio.
[0070] An example of such an isotopic ratio variation parameter is typically is defined
as follows by formula [3]:

where Δt is the time offset applied to the second signal and n is the number of isotope
ratio values for computing the relative standard deviation RSD.
[0071] Alternatively, the isotopic ratio variation parameter can be a combination of both
first a second embodiments.
[0072] The slope-model according to the first embodiment can only be used if a systematic
increase or decrease of the isotopic ratio with time is observed.
[0073] In the case of fast random changes of the isotopic ratio with time due to noisy or
spiky signal behavior, the RSD-model according to the second embodiment is more appropriate
for use.
[0074] According to an eighth step 108, the data collection and processing unit adjusts
the time offset Δt applied to the second signal so as to determine a time offset (Δt
min) for which the isotopic ratio variation parameter is reduced.
[0075] Accordingly, the eighth step 108 can include a modification of the value of the time
offset Δt. The eighth step 108 can then include that the data collection and processing
unit repeats steps 105 to 107 with the new time offset.
[0076] According to the first embodiment, the adjustment step is performed until the slope
S is null or inferior to a pre-determined value. For example, the data collection
and processing unit repeats steps 105 to 108 until the slope S is null or inferior
to 10
-7. Typical slope values after Δt adjustment range from 10
-10 to 10
-16 (isotope ratio/second).
[0077] According to the second embodiment, the adjustment step is performed until the relative
standard deviation RSD raises a minimum or at least has decreased to a value that
is estimated to be close enough to a minimum. For example, the data collection and
processing unit repeats steps 105 to 108 until the relative standard deviation RSD
raises a minimum or at least has decreased to a value that is estimated to be close
enough to a minimum.
[0078] The time offset Δt
min is obtained when isotopic ratio variation parameter raises a minimum or is estimated
to be close enough to a minimum.
[0079] Both isotopic ratio variation parameter (slope S and relative standard deviation
RSD) lead to very similar values of time offset Δt
min. However, the slope-based model is only applicable when a monotonic drift is observed.
The relative standard deviation model may be applied in all cases, even in case of
rapid and random variation of the isotopic ratio, which can be observed when coupling
the mass spectrometer to a laser ablation system.
[0080] Such a time offset Δt
min is applied to the second signal I
b so as to correct the drift in the isotopic ratio I
b/I
a. The method allows computing corrected isotopic ratio values, free from artifacts
caused by detection and amplification systems of the spectrometer.
[0081] The time corrected isotopic ratio values are typically defined by formula 4 as follows:

[0082] In case of N isotopes in the sample (N≥2), the same method is applied to the data
measured for the i-th isotope. A time offset Δt
min is determined for each i-th signal taking one of the signals, for instance the first
signal I
a, as a reference signal.
[0083] According to a ninth step 109, the data collection and processing unit computes a
final value of isotopic ratio as a function of the first signal I
a(t
i) and of the second corrected signal I
b(t
i+Δt
min).
[0084] Several methods can be used to compute the final value of isotopic ratio.
[0085] An average peak method can be applied, wherein the final value of isotopic ratio
is computed as a mean value of the time corrected isotopic ratio values, within a
selected time interval, which can be the same as or different from the time interval
selected at step 104.
[0086] Alternatively, a linear-regression slope method can be applied, wherein a linear
regression of the first signal I
a(t) as a function of the second corrected signal I
b(t+Δt
min) is computed, and the final value of isotopic ratio is calculated as the slope of
the straight line obtained by the linear regression.
[0087] After isotope ratio drift correction both methods give similar results.
EXAMPLE 1: Transient signals with direct injection as introduction system
[0088] The Neptune MC-ICPMS (ThermoFinnigan, Germany) used in this example is equipped with
a multicollector system with nine Faraday cups attached to 10
11 Ohms resistors (dynamic range from 0 Volt to 50 Volts) for simultaneous detection
and provides high mass-resolution capabilities. All measurements were performed in
static multicollection mode with Faraday cups. The Faraday-amplifier gains were calibrated
daily before the analytical session yielding a reproducibility of the electric gains
better than 10 ppm per day. Faraday-amplifier systems have been corrected for compensation
of signal decay (
tau-correction) according to the procedure recommended by the constructor. Intensities
at
m/
z=202 were monitored for eventual
204Hg isobaric interference corrections and found to be inferiors to 0.1milliVolts. All
samples were injected into the plasma through a demountable direct injection high
efficiency nebulizer (d-DIHEN) directly coupled to a flow injection system. The flow
injection system consists of a six-way high flow valve (ESI FAST) with an injection
loop of 5 µL and a peristaltic pump which ensure the continuous flow of the carrier
solution (HNO
3, 0.5N). Cup configuration for Pb measurements and MC-ICPMS operating conditions are
summarized in Table 1.
[0089] All sample dilutions were performed with 0.5 M nitric acid obtained from sub-boiled
14 M nitric acid (EVAPOCLEAN system, Analab, France) and deionised water (Milli Q
system, Millipore, Milford, MA, USA). The same acid was also used as the carrier solution
for the flow injection. For all Pb injections (Neptune-dDIHEN, Nu-GC) the SRM981 standard
solution was used and all calculations were performed by taking into account the isotopic
composition as was reevaluated by Doucelance and Manhès (
Doucelance, R.; Manhès, G. Chemical Geology 2001, 176, 361-377):
208Pb/
206Pb = 2.1681,
207Pb/
206Pb = 0.914970(17),
204Pb/
206Pb = 0.059019(5).
[0090] Pb transient signals were investigated after flow injection and using a demountable
direct injection high efficiency nebulizer (d-DIHEN) as the introduction system in
the Neptune MC-ICPMS. For this purpose, 5 µL of a 100 ppb SRM981 standard solution
were pushed from the carrier solution into the torch. Although flow injection system
has already been used for transient signal studies, the aim of the d-DIHEN is to eliminate
as maximum as possible parameters like memory blanks and processes during generation
and transportation of the aerosol from the spray chamber to the torch. The objective
is therefore to minimize all external parameters which could induce an isotope ratio
fractionation and to highlight isotope ratio drift due to the time lag between the
Faraday-amplifier systems. For transient signal data acquisition an integration time
(
it=0.524 s) longer than the time constant of the Faraday preamplifier response (~0.1
s) was chosen.
[0091] The
208Pb/
206Pb,
207Pb/
206Pb and
204Pb/
206Pb isotope ratios were investigated and only the
208Pb/
206Pb ratio showed a significant drift. As can be seen in Figure 4A the point by point
208Pb/
206Pb isotope ratio shows a systematic increase with time (~0.15%) over a period of ~20
s, which is significantly longer than the time constant of the Faraday-amplifier system.
Therefore, this drift can be attributed to the time lag between H1/H3 (Table 1) Faraday-amplifier
systems.
[0092] For the isotope drift correction the blank-corrected
208Pb and
206Pb intensities with their respective timestamp reads as were recorded from the onboard
computer were used. Blank intensities were calculated for each isotope as the average
value of a time window prior transient signal peak. Before model use, data processing
involves the blank subtraction from each intensity point of
208Pb and
206Pb isotopes.
206Pb isotope is considered as the reference system and timestamp and intensity reads
of
208Pb were used for obtaining the intensity function
I208(
t) by the Piecewise Polynomial Interpolation (PPI) method. In order to be able to efficiently
calculate the time lag (
Δtmin) between H1 and H3 Faraday-amplifiers, the two models were applied in a specific
time-zone where isotope ratio shows a steady trend avoiding high isotope ratio noisy
or spiky behavior (Figure 4A, zone taken into account for the linear regression).
This zone corresponds to
208Pb intensities higher than ~2 Volts. A graphical visualization of the models behavior
as a function of
Δt is given in Figure 4B. As can be seen, Δ
tmin for the
RSD model is slightly shifted toward lower time values compared to the minimum of the
Slope model. Indeed, after
Slope and
RSD models minimization, Δ
tmin values have found to be equal to 0.00165 s and 0.00154 s respectively. Nevertheless,
the
Slope model presents a sharp shape in the minimum region whereas the
RSD model shows a quasi-invariant profile for the same region. Consequently, for
Δt = 0.00165 s, the
RSD model is equal to 0.019785 which is not significantly different compared to the
RSDmin value equal to 0.019725 (obtained for
Δt = 0.00154 s). Thus, it can be considered that Δ
tmin values obtained by models minimization are in good agreement with each other.
[0093] Through equation [5], the calculated time lag can approximately be expressed as the
difference between the stray capacitances of H1 and H3 collector systems which is
called relative stray capacitance.

where τ,
R,
C, are the time constant, the resistor and the capacitor of the Faraday collector system,
Δ
C is denoted the relative stray capacitance between H1 and H3 collector systems, respectively.
[0094] For typical values of
R=10
11 Ω,
C=10
-12 F, τ=0.1 s and Δ
tmin=0.0016 s, Δ
C was found to be equal to 0.016 pF. Therefore, a very small relative stray capacitance
(0.016 pF) between H1 and H3 collector systems induce a time lag in the order of magnitude
of ~0.0016 s which in turn induce a
208Pb/
206Pb isotope ratio drift of ~1.5‰.
[0095] Then, the time corrected
208Pb/
206Pb isotope ratio was calculated using equation [4] and the Δ
tmin value from the
Slope model (Figure 4C). Values of the slope and standard deviation for the selected isotope
ratio zone before and after models correction are given in Table 2. By comparing the
slopes, it can be seen that model efficiently corrects the isotope ratio drift.
[0096] The influence of the signal integration time on the isotope ratio drift was also
investigated. Two independent injections of Pb were performed with 0.262 seconds and
1.049 seconds integration times respectively. For injection with 0.524 seconds integration
time, only the
208Pb/
206Pb isotope ratios showed a significant time dependent drift (Figures 5A et 5C). As
can be seen from Figures 4A, 5A et 5C, a similar trend of the
208Pb/
206Pb isotope ratio drift for the three different integration times was observed. Moreover,
the isotope ratio slopes calculated for the linear regression zones displayed similar
values (Table 2, values of slope before model correction).
[0097] Therefore, it can be concluded that integration time has not a significant influence
on the isotope ratio drift. In contrast, in the same figures it can be observed that
higher integration times lead to smoother
208Pb signal profiles and to smaller isotope ratio random variations. It should be noted
that for transient signals with spiky and nosy shapes (i.e. laser ablation) the use
of relatively long integration times compared to the signal variations (i.e. >0.2
s), could induce inaccurate tracking of the ion signals and consequently can influence
the isotope ratio drift.
[0098] Δ
tmin values were then calculated by the application of the two models in the linear regression
zones (Figures 5A and 5C) and were found to be in good agreement with Δ
tmin values for 0.524 s integration time. Furthermore, like 0.524 s integration time,
Δ
tmin values obtained by the
RSD model were found to be systematically slightly shifted toward lower time values compared
to the
Δtmin of the
Slope model (Table 2). For isotope ratio time correction, the equation [4] and the Δ
tmin values of the
Slope model were used (Figure 5B and 5D).
[0099] Isotope ratio drift correction also highlights the integration time influence on
the % RSD calculated for the linear regression zones. Although higher integration
times lead to smaller isotope ratio random variations, % RSD values before model correction
are dominated by the isotope ratio drift and therefore changes of the integration
time have no significant impact to the %RSD values. In contrast, after isotope ratio
drift correction, it is clear that % RSD for 1.049 s is widely lower than that of
0.262 s (Table 2).
EXAMPLE 2: GC-MC-ICPMS coupling for Pb isotope ratio determination
[0100] The Nu Plasma HR MC-ICPMS (Nu instrument, Wrexham, U.K.) is equipped with twelve
Faraday cups attached to 10
11 Ω resistors for simultaneous detection (dynamic range from 0 V to 10 V). For Pb isotope
ratio measurements, in order to increase the dynamic range of the H4 collector for
208Pb detection, two preamplifiers were connected to the Faraday cup achieving 20 Volts
dynamic range (from -10 V to 10 V). All measurements were performed in static multicollection
mode with Faraday cups. Faraday-amplifier gains were calibrated daily before the analytical
session yielding a reproducibility of the electric gains better than 10 ppm per day.
Tau-correction was performed for all Faraday-amplifier systems. Correction for isobaric
interference on mass 204 was unnecessary firstly because Hg is not present in the
standard solution and secondly Hg species do not elute at the same time as PbEt
4. However,
204Hg presence was monitored using
202Hg and for all injections
202Hg intensities have found to be inferiors to 0.1 milliVolts.
[0101] A commercially double-inlet torch was used for the Gas Chromatography (GC) hyphenation
and the simultaneous introduction of TI solution (200 µL min
-1 of a 200 ng mL
-1 solution) through a self-aspirating microconcentric nebulizer coupled to a cinnabar
spray chamber. Instrumental operation conditions and cup configuration are summarized
in Table 1.
[0102] The developed method for isotope ratio drift correction in transient signals was
applied in data acquired by gas chromatography directly coupled to a Nu MC-ICPMS for
Pb isotope ratio determination. These data consist of thirty independent injections
of a NIST SRM981 standard solution. Data acquisition was performed in static multicollection
mode with an integration time of 0.5 seconds. Elution Pb profiles were highly reproducible
in time, peak-shape and maximum intensity. Typical isotope ratio profiles during Pb
elution are given in Figures 6A to 6C. As can be seen the blank-corrected point by
point isotope ratios showed a negative time drift for
208Pb/
206Pb ratio (decrease with time, ~1.05%) and a positive drift for
207Pb/
206Pb and
204Pb/
206Pb ratios (increase with time, ~0.35% and ~0.17% respectively). Theoretically, in
this case in which a GC issued as the MC-ICPMS introduction system, both chromatographic
separation and time lag between the Faraday-amplifier systems can be considered as
the source of the observed isotope ratio drift. The capillary GC column separates
species by boiling point and thus separation would obey physical laws of isotope mass
fractionation favoring the elution of light isotope masses. Therefore, if the major
source of the observed isotope ratio drifts is mass dependent isotope fractionation
in the GC column,
208Pb/
206Pb and
204Pb/
206Pb ratios should show a positive and negative drift respectively during Pb elution.
Comparing this theoretical consideration with experimental results (Figure 6A and
6C), it is clear that GC mass fractionation cannot be the cause of this drift. Only
207Pb/
206Pb isotope ratio drift is consistent with a possible isotope mass fraction in the
GC column (Figure 6B). In order to shed more light on the source of this drift, the
204Pb/
206Pb and
207Pb/
206Pb isotope ratios were plotted against
208Pb/
206Pb ratios and compared to the Exponential Mass Fractionation Low (EMFL). For these
diagrams, the blank-corrected isotope ratios from the linear regression zones of the
thirty injections were plotted together (Figure 7A and 7B).
[0103] If the observed drifts are caused by a mass-dependent fractionation in the GC column,
the uncorrected data of Figures 7A and 7B should be in good agreement with the EMFL.
Any statistically significant deviation from the EMFL is considered as a mass-independent
fractionation. As can be seen, important deviations from the EMFL clearly point out
that the major source of
204Pb/
206Pb,
207Pb/
206Pb and
208Pb/
206Pb isotope ratio drifts cannot be the isotope mass-dependent fractionation in the
GC column during Pb elution. However, due to the high degree of these deviations (~0.4%),
their origin seems to come more from the instrument (MC-ICPMS) than processes like
nuclear volume and nuclear spin traditionally responsible to mass-independent fractionations.
Therefore, the time lag between the Faraday-amplifier systems is considered as the
major source for explaining this unpredictable behavior of the isotope ratio drifts.
[0104] For the isotope ratio drift correction, the same procedure previously described for
the d-DIHEN introduction system was used. The
206Pb isotope is considered as the reference system and timestamp and intensity reads
of
204Pb,
207Pb and
208Pb isotopes were used for obtaining the intensity functions
I204(t),
I207(
t) and
I208(
t) respectively.
[0105] For each injection, Δ
tmin was calculated by both
the Slope model and the
RSD model. The values were found to be in good agreement each other with Δ
tmin relative differences between the two models of <0.2%, <1% and <4% for the
208Pb/
206Pb,
207Pb/
206Pb and
204Pb/
206Pb ratios respectively. The Δ
tmin values of both models and for the thirty injections are given in Figure 6D. As can
be seen, Δ
tmin of
208Pb/
206Pb and
207Pb/
206Pb ratios have found to be reproducible with average values of -0.0076 ± 2.6% s (2σ)
and 0.00269 ± 8.0% s (2σ) respectively. Negative time lag means that the H4 Faraday-amplifier
system lags behind the H2 reference system (
206Pb isotope). Unlike other the isotope ratios, Δ
tmin values of the
204Pb/
206Pb ratio showed high fluctuations between different injections with an average value
equal to 0.00115 ± 74.6% s (2σ). The large time lag observed for the H4/H2 Faraday
cups could be explained by the use of two amplifiers for increasing the dynamic range
of the H4 collector.
[0106] It should be also noted that, even if time lag between the Faraday-amplifier systems
is the dominant source of the observed isotope ratios drift, mass-dependent isotope
fractionation in the GC column cannot be excluded. Column isotope fractionation generates
an isotope ratio drift that should be added or subtracted to the drift originating
from the Faraday-amplifier time lag (addition for the same slope signs and subtraction
otherwise).
[0107] For the isotope ratio time correction the Δ
tmin values obtained from the
Slope model were used. When comparing the
204Pb/
206Pb,
207Pb/
206Pb and
208Pb/
206Pb slopes of the linear regressions before and after Δ
tmin correction, it appears that isotope ratio drift is efficiently corrected by the model
(Figure 6A, 6B and 6C). Moreover, after drift correction the data much better fit
the EMFL (Figure 7A and 7B).
[0108] The observed dispersion of the corrected data along the EMFL is due to instrumental
mass fractionation changes during the different injection sessions. This is also confirmed
by TI which was continuously introduced into the torch without passing through GC
column. Fractionation factors (β) of
205TI/
203TI and
204Pb/
206Pb,
207Pb/
206Pb,
208Pb/
206Pb ratios reveal identical variations.
Δ204Pb/206Pb and Δ207Pb/206Pb DIAGRAMS
[0109] In order to highlight small deviations of the drift corrected data from the EMFL
(Figure 7A, 7B) at the level of some ppm, representations of Δ
204Pb/
206Pb and Δ
207Pb/
206Pb against
208Pb signal were used (Figure 7C and 7D). Δ
204Pb/
206Pb and Δ
207Pb/
206Pb correspond to the differences between measured and calculated ratios according
to the reference EMFL for a given
208Pb/
206Pb ratio. The
208Pb signal intensity was used in the X-axis due to the continuously changing signal
which significantly influences the counting statistics (Poisson law) and therefore
the isotope ratio precision. As can be seen on Figure 7C, for
208Pb intensities higher than 10 V,
207Pb/
206Pb ratios show downward trend relative to the EMFL with an average value of about
250 ppm. In contrast, for intensities lower than 10 V, the data show a random dispersion
around the EMFL. Different fractionation laws were also used (Power law and Linear
Law) and displayed differences relative to the EMFL which are not distinguishable
for the dispersion of our data. This isotopic deviation from the EMFL has been attributed
to the superposition of the classical mass discrimination isotope evolution (EMFL)
with a non-exponential effect whose physical origin has not been identified yet. Unlike
207Pb/
206Pb,
204Pb/
206Pb results are not conclusive due to the high point dispersion around the EMFL (Figure
7B).
UNCERTAINTIES OF INDIVIDUAL INJECTIONS, REPEATABILITY AND TRUENESS
[0110] The performances of the drift correction on the isotope ratio uncertainty, trueness
and repeatability were also tested and evaluated. The data of the thirty independent
injections of the SRM981 standard solution were treated with the traditionally used
methods for isotope ratio calculation on transient signals; Point by Point (PbP),
Linear Regression (LR) and Peak Area Integration (PAI). The results of the PbP and
LR methods were compared before and after isotope ratio drift correction whereas with
the PAI method only the no drift corrected data were treated. For the PAI method the
integration of 100% of the peak area was selected and therefore time lag between the
Faraday-amplifiers does not have any importance.
[0111] Epov et al. (
Epov, V. N.; Rodriguez-Gonzalez, P.; Sonke, J. E.; Tessier, E.; Amouroux, D.; Bourgoin,
L. M.; Donard, O. F. X. Analytical Chemistry 2008, 80, 3530-3538,
Epov, V. N.; Berail, S.; Jimenez-Moreno, M.; Perrot, V.; Pecheyran, C.; Amouroux,
D.; Donard, O. F. X. Analytical Chemistry 2010, 82, 5652-5662) found that the best isotope ratio precision using the PAI method obtained for an
integration of 90-95% of the peak area. For the measured data, two different integration
zones 95% and 100% of the peak area were tested and no significant differences were
observed. 100% of the peak zone was also used for the LR method and the zone of the
linear regression for the PbP method (Figure 6A, 6B and 6C, isotope ratio zone used
for the linear regression). The blank intensity was calculated for each isotope as
the average value of a zone (duration ~8 s) before the transient signal peak. The
blank contribution was then subtracted from each intensity point of the respective
isotopes. Isotope ratio drifts for all injections were corrected using Δ
tmin values obtained from the
Slope model. The instrumental isotope mass fractionation was corrected internally using
the
208Pb/
206Pb ratio and the exponential mass fractionation low.
[0112] The blank-corrected and mass fractionation-corrected
207Pb/
206Pb,
204Pb/
206Pb isotope ratios treated by different methods before and after isotope ratio drift
correction are presented in Figure 8. Isotope ratio uncertainties for the PbP and
LR methods were calculated for each individual injection by taking into account the
uncertainties of the mass fractionation factor (β
208/206) and of the
207Pb/
206Pb,
204Pb/
206Pb isotope ratios. The latters were calculated as the standard deviation (σ) for the
PbP method and as the slope uncertainty (SE) for the LR method. The SE was calculated
using the command
Regress of
Mathematica and can also be calculated using INDEX(LINEST(...)) function of MS EXCEL. Unlike
PbP and LR methods, PAI method does not provide isotope ratio uncertainties for individual
injections. All isotope ratio uncertainties are expressed for a coverage factor k=2.
[0113] As can be seen, for the PbP method both individual injection uncertainties and repeatability
(σ of thirty injections) of the
204Pb/
206Pb,
207Pb/
206Pb drift corrected ratios were surprisingly improved by a factor 20 and 13 respectively,
compared to the results without drift correction. In contrast, for the isotope ratios
treated with the LR method, repeatability before and after drift correction seems
to be invariant but individual injection uncertainties were improved by a factor 14.
Average values of
204Pb/
206Pb,
207Pb/
206Pb individual injection uncertainties, repeatability and trueness are given in Table
3. As can be seen, contribution of the isotope ratio drift correction to individual
injection uncertainty and to repeatability is most important for the
207Pb/
206Pb ratio due certainly to higher drift compared to that of
204Pb/
206Pb ratio. Drift correction has no statistically significant influence on the average
trueness (trueness of the thirty measurements average); trueness variations are inferior
to the measurement uncertainties, and therefore not significant (Table 3).
TABLE 1: MC-ICPMS and GC operating conditions and Faraday cup configuration
MC-ICPMS conditions |
Neptune |
Nu Plasma |
Sample Introduction System |
|
|
|
GC |
Nebulizer |
d-DIHEN |
Microconcentric (for Tl) |
Spray chamber |
|
|
|
|
|
Cinnabar 20 mL (for Tl) |
Sample gas |
|
|
0.2 (L min-1) |
|
20 (psi) |
|
Ar makeup gas (mL min-1) |
|
|
|
|
|
0.4 |
|
He GC carrier gas (mL min-1) |
|
|
|
|
25 |
|
Liquid uptake (µL min-1) |
50 |
200 (for Tl) |
MC-ICPMS conditions |
|
|
|
|
RF power (W) |
1200 |
1300 |
Plasma gas flow rate (L min-1) |
15 |
13 |
Auxiliary flow rate (L min-1) |
1.3 |
0.9 |
Resolution |
Low |
Low |
Integration time (s) |
0.262, 0.524, 1.049 |
0.5 (TRA mode) |
Sensitivity on 208Pb (V ppm-1) |
120 |
45 |
|
|
|
|
|
|
|
|
|
Cup configuration |
L3 |
L2 |
L1 |
Ax |
H1 |
H2 |
H3 |
H4 |
Neptune |
202Hg |
|
204Pb |
|
206Pb |
207Pb |
208Pb |
|
Nu Plasma |
|
202Hg |
203Tl |
204Pb |
205Tl |
206Ph |
207Pb |
208Pb |
|
|
|
|
|
|
|
|
|
Focus GC |
|
|
|
GC temp. Program |
|
Injector |
Split/splitless |
Initial temperature (°C) |
60 |
Injector volume (µL) |
3 |
Initial time (min) |
2 |
Injector Temperature (°C) |
250 |
Ramp 1 (°C/min) |
60 |
Column |
MXT, 30 m, 0.53 mm i.d., 1.0 mm coating |
Final temperature 1 (°C) |
95 |
|
|
|
|
|
|
Hold time (min) |
5 |
|
|
|
|
|
|
Ramp 2 (°C/min) |
60 |
|
|
|
|
|
|
Final temperature 2 (°C) |
250 |
|
|
|
|
|
|
Hold time (min) |
1 |
TABLE 2: Direct injection - MC-ICPMS Δ
tmin values obtained by the
Slope and
RSD models for different integration times. The values of the slope and the %RSD calculated
for the isotope ratios used for the linear regression were also presented.
Int. Time (s) |
Δtmin (s) |
|
Values of slope |
|
Values of% RSD |
|
Slope model |
RSD model |
|
No corrected |
Corrected |
|
No corrected |
Corrected |
0.262 |
0.00161 |
0.00151 |
|
1.14×10-4 |
4.93×10-11 |
|
0.0318 |
0.0208 |
0.524 |
0.00165 |
0.00154 |
|
8.95×10-5 |
4.20×10-16 |
|
0.0295 |
0.0197 |
1.049 |
0.00163 |
0.00157 |
|
8.33×10-5 |
6.68×10-14 |
|
0.0273 |
0.0132 |
|
|
|
|
|
|
|
|
|
TABLE 3: GC-MC-ICPMS average values of
207Pb/
206Pb and
204Pb/
206Pb isotope ratios uncertainty, repeatability and trueness of no corrected and corrected
data for isotope ratio drift. Where PbP, LR and PAI are the Point by Point, the Linear
Regression and the Peak Integration methods respectively. Uncertainties and repeat
abilities are expressed for a coverage factor k=2.
207Pb/206Pb |
PbP |
|
LR |
|
PAI |
|
No corrected |
Corrected |
|
No corrected |
Corrected |
|
No corrected |
% Uncertainty |
0.50 |
0.024 |
|
0.034 |
0.0024 |
|
|
% Repeatability 0.098 |
|
0.0072 |
|
0.0062 |
0.0062 |
|
0.0058 |
% Trueness |
0.030 |
0.014 |
|
0.018 |
0.019 |
|
0.016 |
|
|
|
|
|
|
|
|
204Pb/206Pb |
|
|
|
|
|
|
|
% Uncertainty |
0.52 |
0.088 |
|
0.031 |
0.017 |
|
|
% Repeatability |
0.125 |
0.034 |
|
0.022 |
0.022 |
|
0.062 |
% Trueness |
0.013 |
0.032 |
|
0.030 |
0.030 |
|
0.025 |
|
|
|
|
|
|
|
|
1. Method for correcting a drift of an isotopic ratio in a sample, on the basis of a
first signal (I
a) and a second signal (I
b) derived from data measured by a multi-collector mass spectrometer, the first signal
(I
a) representing a variation of a detected quantity of a first isotope (a) in the sample
as a function of time, and the second signal (I
b) representing a variation of a detected quantity of a second isotope (b) in the sample
as a function of time, said method comprising steps of:
- applying (105) to the second signal (Ib) a time offset (Δt) so as to obtain a second offset signal (Ib(t+Δt)),
- computing (106) values of isotopic ratio between the first signal (Ia) and the second offset signal (Ib(t+Δt)) at a plurality of times (ti),
- computing an isotopic ratio variation parameter as a function of the computed values
of isotopic ratio,
- adjusting the time offset (Δt) applied to the second signal (Ib) and repeating the preceding steps so as to determine a time offset (Δtmin) for which the isotopic ratio variation parameter is reduced.
2. Method according to claim 1, comprising a step of:
- computing the second signal (Ib(t)) by interpolation of second data representing detected quantities of a second
isotope (b), measured in the sample at different times.
3. Method according to claim 2, wherein the interpolation is a piecewise polynomial interpolation.
4. Method according to one of claims 1 to 3, wherein the steps are applied to a number
N of signals, N>2, each i-th signal representing a variation of a detected quantity
of a i-th isotope in the sample as a function of time, so as to determine a time offset
for each of the second to the N-th signals.
5. Method according to one of claims 1 to 4, wherein the isotopic ratio variation parameter
is a slope of a straight line obtained by linear regression of the values of isotopic
ratio.
6. Method according to one of claims 1 to 4, wherein the isotopic ratio variation parameter
is a relative standard deviation of the values of isotopic ratio.
7. Method according to one of claims 1 to 6, comprising a step of:
- selecting a time interval in which the values of isotopic ratio are computed.
8. Method according to one of claims 1 to 6, wherein the steps are carried out on several
time intervals, and a time offset is determined for each time interval.
9. Method according to one of claims 1 to 8, comprising preliminary steps of:
- introducing a sample into the multi-collector mass spectrometer, and
- measuring data from the sample, the data being measured by the spectrometer.
10. Method according to claim 9, wherein the multi-collector mass spectrometer is coupled
to a separation system for separating the sample into several elementary fractions
and successively introducing the elementary fractions into the spectrometer.
11. Method according to claim 10, wherein the separation system is a liquid, high performance
liquid, ionic or a gas chromatography system.
12. Method according to claim 10, wherein the multi-collector mass spectrometer is coupled
to a laser ablation system for in situ analysis of solid materials or single micrometric
particle size analysis, so as to obtain the sample to be introduced into the multi-collector
mass spectrometer.
13. Method according to one of claims 1 to 12, wherein the multi-collector mass spectrometer
comprises an ion source selected from the group consisting in a thermal ionization
device, an electron ionization device and a plasma ionization device.
14. Method according to one of claims 1 to 13, wherein the multi-collector mass spectrometer
is a multi-collector inductively coupled plasma mass spectrometer.
15. Processing unit adapted for receiving data measured on a sample by a multi-collector
mass spectrometer, and configured for correcting a drift of an isotopic ratio in the
sample according to the method defined by one of claims 1 to 14.
16. Computer program for correcting a drift of an isotopic ratio in a sample from data
measured on the sample by a multi-collector mass spectrometer, comprising program
instructions for causing a processing unit to implement the method defined by one
of claims 1 to 14.